Titlebook: Coronal Expansion and Solar Wind; A. J. Hundhausen Book 1972 Springer-Verlag Berlin · Heidelberg 1972 Korona (Astron.).Orbit.Scale.Sonnenw

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II–VI electroluminescent deviceservations of a continuous supersonic flow of plasma and a magnetic field configuration fitting the expected pattern by the first spacecraft to probe interplanetary space demonstrated the fundamental validity of this concept and theory.

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Bulk growth of widegap II–VI single crystalsr ambient solar wind (such as already shown in Fig. 5.9). Fig. 6.1 shows a hypothetical cross section (in the solar equatorial plane) of the resulting solar wind disturbance at a time when it has traveled well out into interplanetary space.

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Book 1972ons con- firmed the basic validity of a theoretical model, first proposed by E. N. Parker, predicting a continuous, rapid expansion of the solar corona. The subsequent decade has seen a tremendous growth in both the breadth and sophistication of solar wind observations; the properties of the interpl

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Chemical Composition of the Expanding Coronal and Interplanetary Plasma, the polarization electric field of the coronal plasma, as already described in I.6. Ions other than .H. and .H. can be observed by present day plasma detectors only under favorable (and rare) circumstances. These infrequent observations have led to some knowledge of the interplanetary abundance of